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@ARTICLE{Kumaran:897149,
author = {Kumaran, Sindhujha and Ludhova, Livia and Penek, Ömer and
Settanta, Giulio},
title = {{B}orexino {R}esults on {N}eutrinos from the {S}un and
{E}arth},
journal = {Universe},
volume = {7},
number = {7},
issn = {2218-1997},
address = {Basel},
publisher = {MDPI},
reportid = {FZJ-2021-03639},
pages = {231 -},
year = {2021},
abstract = {Borexino is a 280-ton liquid scintillator detector located
at the Laboratori Nazionali del Gran Sasso in Italy. Since
the start of its data-taking in May 2007, it has provided
several measurements of low-energy neutrinos from various
sources. At the base of its success lie unprecedented levels
of radio-purity and extensive thermal stabilization, both
resulting from a years-long effort of the collaboration.
Solar neutrinos, emitted in the Hydrogen-to-Helium fusion in
the solar core, are important for the understanding of our
star, as well as neutrino properties. Borexino is the only
experiment that has performed a complete spectroscopy of the
pp chain solar neutrinos (with the exception of the hep
neutrinos contributing to the total flux at 10$^{−5}$
level), through the detection of pp, $^7$Be, pep, and $^8$B
solar neutrinos and has experimentally confirmed the
existence of the CNO fusion cycle in the Sun. Borexino has
also detected geoneutrinos, antineutrinos from the decays of
long-lived radioactive elements inside the Earth, that can
be exploited as a new and unique tool to study our planet.
This paper reviews the most recent Borexino results on solar
and geoneutrinos, from highlighting the key elements of the
analyses up to the discussion and interpretation of the
results for neutrino, solar, and geophysics.},
cin = {IKP-2},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000677070100001},
doi = {10.3390/universe7070231},
url = {https://juser.fz-juelich.de/record/897149},
}